Modelling the anisotropic two-point galaxy correlation function on small scales and single-probe measurements of H(z), DA(z) and f(z)σ8(z) from the Sloan Digital Sky Survey DR7 luminous red galaxies
292 citations recorded by the source corpus.
We present a simple and efficient phenomenological model for the two-dimensional two-point galaxy correlation function that works well over a wide range of scales, from large scales down to scales as small as 25Mpc/h. Our model incorporates nonlinear effects, a scale-dependent galaxy bias on small scales, and allows the redshift-space distortions to be scale and direction dependent. We validate our model using LasDamas mock catalogs, and apply it to the Sloan Digital Sky Survey (SDSS) DR7 Luminous Red Galaxies (LRGs). Using only the monopole and quadrupole of the correlation function measured from the SDSS DR7 LRGs, we obtain improved measurements H(z)r_s(z_d)/c=0.0433\pm 0.0042, D_A(z)/r_s(z_d)=6.59\pm 0.46, and f(z)sigma_8(z)=0.429\pm 0.089 at z=0.35, using the scale range of 25<s<120Mpc/h. We expect our results and model to be useful in tightening dark energy and gravity constraints from the full analysis of current and future galaxy clustering data.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/150ad6d7be9e7cc2e9536404822dff73d3e4a65a
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In Astronomy and Astrophysics
- D. Schneider
- Daniel J. Eisenstein
- C. Chuang
- J. Brownstein
- Will J. Percival
- A. Ross
- K. Dawson
- David Schlegel
In Nuclear and High Energy Physics
- C. Chuang
- D. Schneider
- L. Perivolaropoulos
- Daniel J. Eisenstein
- S. Nesseris
- David Schlegel
- A. Ross
- Marc Manera
Citations in the corpus
- The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from CMASS anisotropic galaxy clustering (2013, methodology): “This task is efficiently performed by using Legendre polynomial expansions and one-dimensional integral convolutions as introduced in Chuang & Wang (2013b).”
- Evolution of the f σ 8 tension with the Planck 15 / Λ CDM determination and implications for modified gravity theories (2018, background): “[84] Chia-Hsun Chuang and Yun Wang, “Modelling the”
- Tension and constraints on modified gravity parametrizations of $G_{\textrm{eff}}(z)$ from growth rate and Planck data (2017, background): “[63] Chia-Hsun Chuang and Yun Wang, “Modeling the Anisotropic Two-Point Galaxy Correlation Function on Small Scales and Improved Measurements of H(z), DA(z), and β(z) from the Sloan Digital Sky Survey DR7 Luminous Red Galaxies,” Mon.”
- HUBBLE PARAMETER MEASUREMENT CONSTRAINTS ON THE REDSHIFT OF THE DECELERATION–ACCELERATION TRANSITION, DYNAMICAL DARK ENERGY, AND SPACE CURVATURE (2016, result): “We drop older SDSS galaxy clustering H(z) determinations from Chuang & Wang (2013) in favor of the more recent measurements from Alam et al. (2016).”